Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2301.03825.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T13:29:57.722782Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 6f718d8b-68a9-4456-8f82-960d1d382402 · inbound
From Streaming Instability to the Onset of Pebble Accretion I. Investigating the Growth Modes in Planetesimal Rings cites this paper.
From Streaming Instability to the Onset of Pebble Accretion I. Investigating the Growth Modes in Planetesimal Rings An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T13:29:57.722782Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 77fce80d-2ca9-429a-b8e8-02f455c6477f · inbound
Where are the missing Kuiper Belt binaries? cites this paper.
Where are the missing Kuiper Belt binaries? An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:16:16.477280Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fc5b8943-5270-47ce-bb95-479d9552dc07 · inbound
Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets cites this paper.
Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion
Reference 48
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T03:28:01.085344Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 74528c50-5b54-4c41-a706-cfd4f8a92e4f · inbound
Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets cites this paper.
Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T13:48:34.799680Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 45e26807-fa0c-41ee-a1a6-a066ff80f06a · inbound
Dust and Gas Transport in Substructured Nonideal MHD Wind-Launching Disks with Embedded Planets cites this paper.
Dust and Gas Transport in Substructured Nonideal MHD Wind-Launching Disks with Embedded Planets An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion
Reference 172
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T10:42:18.267921Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.